Hubble Space Telescope Spectroscopy of the Nucleus of M33

Details Hubble Space Telescope Spectroscopy of the Nucleus of M33 Hubble Space Telescope Spectroscopy of the Nucleus of M33

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002apj...569..204l&link_type=abstract

The Astrophysical Journal, Volume 569, Issue 1, pp. 204-213.

Astronomy and Astrophysics

Astronomy

24

Galaxies: Individual: Messier Number: M33, Galaxies: Nuclei, Galaxies: Stellar Content, Galaxies: Local Group, Ultraviolet: Stars

Scientific paper

We have used the Hubble Space Telescope to obtain moderate resolution 1150-5700 Å spectroscopy of the nucleus of M33 and a blue star ~1" north-northwest of the nucleus in an attempt to find the optical counterpart of the nuclear X-ray source and to characterize stellar populations in the nuclear region. The Space Telescope Imaging Spectrograph spectra of the nucleus can be modeled in terms of two starbursts: one with a mass of about 9000 Msolar at 40 Myr and the other with a mass of about 76,000 Msolar at 1 Gyr. The blue star is a late-type O giant with no obvious spectral anomalies to indicate that it is associated with the luminous X-ray source. The nuclear region is not heavily reddened; 2200 Å absorption features in the spectra of both the nucleus and the star are weak. The data and the star formation history support the hypothesis that the M33 nuclear source, the brightest persistent source in the Local Group, is an ~10 Msolar black hole binary. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with proposal 8341.

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